Theory Observation
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Moon and Planetary Nomenclatures
Planetary nomenclature became in 1919 the exclusive domain of the International Astronomical Union (IAU) which had been founded this very year in Brussels. IAU took back previous works of regularization about naming Moon and Mars features. Final works about Moon were published in 1936, (Miss Blagg and Muller) then in the 1965s (Gerard K. Kuiper) as Martian nomenclature was stabilized about 1960 only (Audouin Dollfus), building upon previous nomenclatures by Schiaparelli and Antoniadi. Space exploration produced new needs for nomenclature for Moon and planets of the solar system and their moons (1970s works of Gerard de Vaucouleurs and Donald H. Menzel). Since that time IAU has a Working Group for Planetary System Nomenclature (WGPSN) and diverse task groups. A theme is choosen for each celestial body, names are decided along the theme by the task group as investigators of the body then propose additional names. Names accepted by a task group and successfully submitted to the WGPSN are considered provisionally approved until they are eventually officially accepted by the IAU's General Assemby meeting each three years. see more at the Planetary System Nomenclature (WGPSN)'s page, which is hosted at the U.S. Geological Survey (USGS) Rules for the naming of satellites of the solar system planets are the following:
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